Chandrasekhar potential energy tensor

In astrophysics, Chandrasekhar potential energy tensor provides the gravitational potential of a body due to its own gravity created by the distribution of matter across the body, named after the Indian American astrophysicist Subrahmanyan Chandrasekhar.[1][2][3] The Chandrasekhar tensor is a generalization of potential energy in other words, the trace of the Chandrasekhar tensor provides the potential energy of the body.

Definition

The Chandrasekhar potential energy tensor is defined as

where

where

It is evident that is a symmetric tensor from its definition. The trace of the Chandrasekhar tensor is nothing but the potential energy .

Hence Chandrasekhar tensor can be viewed as the generalization of potential energy.[4]

Chandrasekhar's Proof

Consider a matter of volume with density . Thus

Chandrasekhar tensor in terms of scalar potential

The scalar potential is defined as

then Chandrasekhar[5] proves that

Setting we get , taking Laplacian again, we get .

See also

References

  1. Chandrasekhar, S; Lebovitz NR (1962). "The Potentials and the Superpotentials of Homogeneous Ellipsoids" (PDF). Ap. J. 136: 1037–1047. Bibcode: 1962ApJ...136.1037C. doi:10.1086/147456. Retrieved March 24, 2012.
  2. Chandrasekhar, S; Fermi E (1953). "Problems of Gravitational Stability in the Presence of a Magnetic Field" (PDF). Ap. J. 118: 116. Bibcode: 1953ApJ...118..116C. doi:10.1086/145732. Retrieved March 24, 2012.
  3. Chandrasekhar, Subrahmanyan. Ellipsoidal figures of equilibrium. Vol. 9. New Haven: Yale University Press, 1969.
  4. Binney, James; Tremaine, Scott. Galactic Dynamics: (Second Edition). Princeton University Press. pp. 59–60. ISBN 1400828724.
  5. Chandrasekhar, Subrahmanyan. Ellipsoidal figures of equilibrium. Vol. 9. New Haven: Yale University Press, 1969.
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